SIMBAD references

2008A&A...483L...9V - Astronomy and Astrophysics, volume 483, L9-12 (2008/5-3)

Is the silicate emission feature only influenced by grain size?

VOSHCHINNIKOV N.V. and HENNING T.

Abstract (from CDS):

The flattening of the 10µm silicate emission feature observed in the spectra of T Tauri and Herbig Ae/Be stars is usually interpreted as an indicator of grain growth. We show in this paper that a similar behaviour of the feature shape occurs when the porosity of composite grains varies. We modelled the fluffy aggregates with inclusions of different sizes with multi-layered spheres consisting of amorphous carbon, amorphous silicate, and vacuum. We also found that the inclusion of crystalline silicates in composite porous particles can lead to a shift of the known resonances and production of new ones.

Abstract Copyright:

Journal keyword(s): line: profiles - stars: pre-main-sequence - stars: planetary systems: protoplanetary disks - stars: circumstellar matter - infrared: stars - ISM: dust, extinction

CDS comments: Table 1 star Tr 37 01-580 is a misprint for [SHB2004] NGC 7160 01-580.

Simbad objects: 49

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2020.10.30-14:28:56

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